Line Formation in the Inner Starburst Regions of AGN

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We review the evidence for young stellar populations in the inner (< 200 pc) regions of Active Galactic Nuclei (AGN), and the physical mechanisms through which the stars can potentially create the emission lines that characterize AGN.
Invited talk in 'Winds, Bubbles and Explosions' (Patzcuaro, Mexico, Sep. 2002), 6 pages, 3 figures

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/5775

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0302442
 http://arxiv.org/abs/astro-ph/0302442
 2003, RevMexAA Conf. Ser., 15, 329

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arXiv